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Title: Alpha Decay of 109I and the Implications for the Rapid-Proton Capture Process

Conference ·
OSTI ID:946106
 [1];  [2];  [3];  [4];  [3];  [5];  [1];  [2];  [4];  [6];  [6];  [7];  [1];  [8];  [9];  [10];  [1]
  1. University of Tennessee, Knoxville (UTK)
  2. University of Tennessee
  3. Michigan State University, East Lansing
  4. ORNL
  5. Oak Ridge Associated Universities (ORAU)
  6. Vanderbilt University
  7. Mississippi State University (MSU)
  8. University of Warsaw
  9. Joint Institute for Heavy Ion Research, Oak Ridge
  10. University of Liverpool

In an experiment at the Recoil Mass Spectrometer of the HRIBF at ORNL the alpha decay branch of {sup 109}I was discovered. The measurement of its decay energy allowed for the indirect determination of the proton separation energy in the daughter nucleus {sup 105}Sb. The deduced S{sub p}({sup 105}Sb) = -356(22) keV is about 130 keV larger than the previously claimed value. The consequences of this measurement for the astrophysical rp-process will be discussed.

Research Organization:
Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
Sponsoring Organization:
USDOE Office of Science (SC)
DOE Contract Number:
DE-AC05-00OR22725
OSTI ID:
946106
Resource Relation:
Conference: Tenth International Symposium on Nuclei in the Cosmos (NIC-X), Mackinac Island, MI, USA, 20080727, 20080801
Country of Publication:
United States
Language:
English